Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Matter ejections behind the highs and lows of the transitional millisecond pulsar PSR J1023+0038
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2305.14509.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.611206Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
1
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 902d2e34-6f43-4517-9c5a-7064731d7b8c · inbound
Fast optical spectroscopic observations of PSR J1023+0038 over one orbital period cites this paper.
Fast optical spectroscopic observations of PSR J1023+0038 over one orbital period Matter ejections behind the highs and lows of the transitional millisecond pulsar PSR J1023+0038
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T02:10:32.260915Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f7777995-7031-45cc-99b4-a5650486a308 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry Matter ejections behind the highs and lows of the transitional millisecond pulsar PSR J1023+0038
Reference 210
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-07T20:40:58.228634Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.